HALO - I. Photometric continuum reverberation mapping of Fairall 9

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Table 1.

Basic properties of Fairall 9.

z	log L_AGN, 5100	F_AGN, 5100 (1 + z)	τ_cent, Hβ	σ_line, Hβ	FWHM	M_BH	log λ_Edd	i
	(erg s⁻¹)	(× 10⁻¹⁵ erg s⁻¹ cm⁻² Å⁻¹)	(days)	(km s⁻¹)	(km s⁻¹)	(×10⁸ M_⊙)		(degree)
(1)	(2)	(3)	(4)	(5)	(6)	(7)	(8)	(9)
0.046145	43.92 ± 0.05^(a)	2.95 ± 0.23^(a)	$17 . 4_{- 4.3}^{+ 3.2 (b)}$ $17.4_{-4.3}^{+3.2\,(b)}$	3787 ± 197^(b)	6901 ± 707^(b)	2.18 ± 0.46	−1.551 ± 0.104	$35 . 0_{- 5.6}^{+ 3.4 (c)}$ $35.0_{-5.6}^{+3.4\,(c)}$

Notes. The columns are as follows: (1) redshift z, (2) AGN luminosity at 5100 Å, (3) AGN monochromatic flux at 5100 Å, (4) Hβ BLR lag in rest-frame, (5) Hβ line dispersion, (6) FWHM of Hβ line, (7) black hole mass measured from τ_cent, Hβ and σ_line, Hβ with virial factor f_BLR = 4.47 (Woo et al. 2015), (8) logarithm of Eddington ratio, and (9) inclination angle. References are (a) Bentz et al. (2013), (b) Peterson et al. (2004), and (c) Lohfink et al. (2012).

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